Dynamics of local dust clumps in a protostellar cloud

Details Dynamics of local dust clumps in a protostellar cloud Dynamics of local dust clumps in a protostellar cloud

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985azh....62..711k&link_type=abstract

(Astronomicheskii Zhurnal, vol. 62, July-Aug. 1985, p. 711-718) Soviet Astronomy (ISSN 0038-5301), vol. 29, July-Aug. 1985, p. 4

Statistics

Computation

Cosmic Dust, Gas Dynamics, Interstellar Gas, Protostars, Clumps, Computational Astrophysics, Equations Of Motion, Temporal Distribution

Scientific paper

The time scales for compact aggregates of solid matter to condense from loose local clumps of dust grains in a protostellar cloud are determined by numerically solving the equations describing the clump dynamics. The results indicate that dense aggregates of dust can form in a protostellar cloud by a process which has nothing to do with gravitational instability effects. Thus, dense bodies can form from micron-size particles.

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